mary hudson. functions. Space Physicist Mary K. Hudson, PhD UCLA 1974, is Professor of Physics and served for eight years as Chair of Physics and Astronomy at Dartmouth College. Senior Research Associate, NCAR High Altitude Observatory Space Physicist Mary K. Hudson, PhD UCLA 1974, is Professor of Physics and served for eight years as Chair of Physics and Astronomy at Dartmouth College. She has served as chair of the NSF Geospace Environment Modeling program and has been an Advanced Study Program Visitor and now Affiliate Scientist at the High Altitude Observatory, National Center for Atmospheric Research, and hosted by the UC Berkeley Space Sciences Laboratory and the University of Colorado Laboratory for Atmospheric and Space Physics.

She has served as chair of the NSF Geospace Environment Modeling program and has been an Advanced Study Program Visitor and now Affiliate Scientist at the High Altitude Observatory, National Center for Atmospheric Research, and hosted by the UC Berkeley Space Sciences Laboratory and the University of Colorado Laboratory for Atmospheric and Space Physics. secretaries, respectively, and Bruce Tsurutani is the new

Simulations Res., 112, A09215, doi:10.1029/2006JA012218.Kress, B.T., M K Hudson and P L Slocum Impulsive Solar Energetic Ion Trapping in the Magnetosphere During Geomagnetic storms, Geophys. It is shown that there is little difference between having a finite temperature in the electron beam and leaving the beam cold. The fundamental electromagnetic nature of the interchange mode is noted: coupling to the intermediate Alfven mode is strongly stabilizing for finite pert...The structure of the drift instability is examined in several density regimes.

Mary Hudson. Professor Hudson is also funded through NSF to study solar energetic particles and their access to the atmosphere.Along with students and postdoctoral research staff, Professor Hudson is modeling sudden changes in relativistic electron fluxes at and inside the 24-hr orbital period of many communication and navigation satellites, which are affected by global oscillations of the Earths magnetic field, associated with changes in solar wind conditions which have their origins at the sun. Hudson and her students study the weather patterns that originate from solar eruptions, following the energy and mass transfer through the interplanetary medium, all the way to the earth's ionosphere. Biographical Sketch – Mary K. Hudson mary.hudson@dartmouth.edu; Eleanor and A. Kelvin Smith Professor of Physics Department of Physics and Astronomy Dartmouth College, Hanover NH 03755 (a) Professional Preparation UCLA Physics Ph.D., 1974 UCLA Physics M.S., 1971 UCLA Physics B.S., 1969 (b) Appointments 1969-71, Associate Staff, Space Sciences Lab, The Aerospace Corporation, El Segundo … Eleanor and Kelvin Smith Distinguished Professor of PhysicsSenior Research Associate, NCAR High Altitude Observatory We evaluate both the average transport coefficients used in quasi-linear diffusion transport and also the full...The mechanisms that drive relativistic electron precipitation (REP) from the radiation belts can be better understood with a better knowledge of the particle energies involved.

Electric field fluctuations have been ob...A fluid dispersion relation for the drift and interchange (Rayleigh-Taylor) modes in a collisional plasma forms the basis for a linear theory of equatorial spread F. The collisional-drift-mode growth rate will exceed the growth rate of the Rayleigh-Taylor mode at short perpendicular wavelengths and density-gradient scale lengths. Home. simulations. The High Altitude Observatory (HAO) of the National Center for Atmospheric research (NCAR) is located in Boulder, Colorado, at the foot of the … Res.

Magnetospheric Physics, and Solar and Heliospheric Physics section Vince Mary Hudson and her colleagues, William Lotko (left) and John Lyon (center), want to find better ways to predict storms in space.

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